PPT-MAGNITUDES

MAGNITUDES Magnitudes son las cualidades o propiedades de los seres o sucesos que se pueden medir Long circunferencia 68 73  cm Longitud diámetro 2324 cm M asa . ed(#)d#㲓75% of blue counts"r g468140-0.08V550800r617140+0.14RC6601600R7002200i748150+0.34IC810 Magnitudes from differ UCERF2. and . Plans for UCERF3. Andy Michael. Historical Earthquake Catalog: 1850 – 1932. Primary compilation: . Toppozada. and . Branum. (2003). 1769-1999, M≥5.5, magnitude based on area with MMI V, VI, VIII,. A escala de magnitude Richter não tem unidade e não tem limite superior ou inferior de valor. Ela foi desenvolvida apenas para efeito de comparação relativa entre sismos. Ela não é uma medida direta da energia liberada pelo sismo, nem do tamanho da área de ruptura do sismo. No entanto, é possível relacionar, empiricamente, a magnitude com outros parâmetros físicos do sismo. Um exemplo de relação entre magnitude e energia, é dada por:. Announcements. This week: Dark Night Observing . tonight. First “Astro-group” meeting. - Friday, 9/11; 2:30-3:30 E-109. Definitions & Terms -1. Photometric Conditions:. Differential Photometry. Calculating magnitudes from AS-1 seismograms (electronic version) 1 (L. Braile braile@purdue.edu www.eas.purdue.edu/~braile 1. Introduction: This education module is designed to provide experienc Empezar. . de nuevo. Lee detenidamente las magnitudes eléctricas y responde a las cuestiones posteriores. Cada cuestión fallada te traerá de nuevo a esta página y deberás empezar de nuevo. Presta atención. getting ready for our (any!) observing run. http://cheezburger.com/5797953792. http://glozing.blogspot.com/2012/09/like-scouts-say-be-prepared.html. http://. labasslix.com. /be-prepared/. YOU THE OBSERVER should never be the cause of this:. 1 From upernovae , their Light - Curves, and Angular Sizes of Galaxies to a Tenable Cosmology Hartmut Traunm 25 years of Astronomy. Etteyeb Nejmeddine. 21 years old. The Astronomical Society of Tunisia (SAT) . The Charlie Bates Solar Astronomy Project (CBSAP). Computer Science . What Are Variable Stars?. Detecting variability. Chapter 17. How do stars differ? Is . the Sun typical?. Image . of Orion illustrates:. The huge number of stars. Colors. Interstellar . gas. How can we describe/classify stars. ?. Location. Temperature. A Research Project by Dominic Elizondo. Contrasting Open and Globular Clusters. Age. Location. Number of Stars. M2 Globular Cluster. M11 Open Cluster. Data Collection. 20’’ f/6.8 Plane Wave . Cassegrain. cyg. . A Project by andy parker. Background. Cataclysmic Variable stars are binary star pairs consisting of a white dwarf and red giant star (usually).. The white dwarf star rips away its stair pair’s matter because its gravitational pull is much greater than that of its partner.. Today’s Concepts:. . A) Electric Flux. B) Field Lines. Gauss’ Law. Unit . 3, Slide . 1. Electric Field Lines. Unit . 3, Slide . 2. . Q. First….a comment. What the point of all this flux stuff?. L. B. >L. A. =L. F. =L. G. >L. E. >L. C. >L. D. L. C. =L. B. =L. A. =L. D. >L. E. =L. F. >L. G. L. A. >L. B. =L. C. =L. D. >L. E. >L. F. >L. G. L. B. >L. A. =L. C. =L.